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Development of a space-borne spectrometer to monitor atmospheric ozone.

作者信息

Dobrolenskiy Yury S, Ionov Dmitry V, Korablev Oleg I, Fedorova Anna A, Zherebtsov Evgeny A, Shatalov Andrey E, Mantsevich Sergey N, Belyaev Denis A, Vyazovetskiy Nikita A, Moiseev Pavel P, Tchikov Konstantin N, Krasavtsev Valery M, Savushkin Alexander V, Rumyantsev Dmitry M, Kananykhin Igor V, Viktorov Alexey I, Kozyura Alexey V, Moryakin Sergey A, Poberovskii Anatoly V

出版信息

Appl Opt. 2015 Apr 10;54(11):3315-22. doi: 10.1364/AO.54.003315.

DOI:10.1364/AO.54.003315
PMID:25967319
Abstract

A new compact satellite spectrometer dedicated to monitoring terrestrial atmospheric ozone (ozonometer) is in preparation for the Russian Geophysics Program. Four instruments at four satellites (Ionosphere) are intended to monitor the total ozone content by measuring spectra of scattered solar radiation in nadir. The spectrometer is based on the Rowland scheme with a concave holographic diffraction grating. It covers the near UV and visible range of the spectrum, 300-500 nm, with a spectral resolution of ∼0.3  nm. At present, a qualification model has been manufactured and tested. We introduce the description of the instrument and the results of laboratory and ground-based atmospheric calibrations. The ozone amount retrieved from atmospheric measurements using the differential optical absorption spectroscopy (DOAS) method is in good agreement with that measured by the collocated Brewer spectrophotometer and ozone monitoring instrument on board the Aura satellite.

摘要

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